The nature of H α-selected galaxies along the large-scale structure at z = 0.4 revealed by Subaru Hyper Suprime-Cam survey-Reference-Cited by-同舟云学术

The nature of H α-selected galaxies along the large-scale structure at z = 0.4 revealed by Subaru Hyper Suprime-Cam survey

Published:2017-09-06 Issue:SP1 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Koyama Yusei¹²,Hayashi Masao³,Tanaka Masayuki³,Kodama Tadayuki³⁴,Shimakawa Rhythm⁵,Yamamoto Moegi²,Nakata Fumiaki¹,Tanaka Ichi¹,Suzuki Tomoko L³,Tadaki Ken-ichi³,Nishizawa Atsushi J⁶,Yabe Kiyoto⁷,Toba Yoshiki⁸,Lin Lihwai⁷,Jian Hung-Yu⁷,Komiyama Yutaka³²

Affiliation:

1. Subaru Telescope, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 650 North A’ohoku Place, Hilo, HI 96720, USA

2. Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

3. National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

4. Astronomical Institute, Tohoku University, 63 Aramaki, Aoba-ku, Sendai, Miyagi 980-8578, Japan

5. UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064, USA

6. Institute for Advanced Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan

7. Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan

8. Academia Sinica Institute of Astronomy and Astrophysics, PO Box 23-141, Taipei 10617, Taiwan

Funder

National Aeronautics and Space Administration

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/SP1/S21/23692301/psx078.pdf

Reference105 articles.

1. DIFFERENCES IN THE STRUCTURAL PROPERTIES AND STAR FORMATION RATES OF FIELD AND CLUSTER GALAXIES AT Z ∼ 1

2. Galaxy And Mass Assembly (GAMA): stellar mass growth of spiral galaxies in the cosmic web

3. Galaxy bimodality versus stellar mass and environment

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